Bubble Formation in Magma

IF 11.3 1区 地球科学 Q1 ASTRONOMY & ASTROPHYSICS
J. Gardner, F. Wadsworth, T. Carley, E. Llewellin, H. Kusumaatmaja, D. Sahagian
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引用次数: 7

Abstract

Volcanic eruptions are driven by bubbles that form when volatile species exsolve from magma. The conditions under which bubbles form depend mainly on magma composition, volatile concentration, presence of crystals, and magma decompression rate. These are all predicated on the mechanism by which volatiles exsolve from the melt to form bubbles. We critically review the known or inferred mechanisms of bubble formation in magmas: homogeneous nucleation, heterogeneous nucleation on crystal surfaces, and spontaneous phase separation (spinodal decomposition). We propose a general approach for calculating bubble nucleation rates as the sum of the contributions from homogeneous and heterogeneous nucleation, suggesting that nucleation may not be limited to a single mechanism prior to eruption. We identify three major challenges in which further experimental, analytical, and theoretical work is required to permit the development of a general model for bubble formation under natural eruption conditions. ▪ We review the mechanisms of bubble formation in magma and summarize the conditions under which the various mechanisms are understood to operate. ▪ Bubble formation mechanisms may evolve throughout magma ascent as conditions change such that bubbles may form simultaneously and sequentially via more than one mechanism. ▪ Contributions from both homogeneous nucleation and heterogeneous nucleation on multiphase crystal phases can be captured via a single equation. ▪ Future work should focus on constraining macroscopic surface tension, characterizing the microphysics, and developing a general framework for modeling bubble formation, via all mechanisms, over natural magma ascent pathways. Expected final online publication date for the Annual Review of Earth and Planetary Sciences, Volume 51 is May 2023. Please see http://www.annualreviews.org/page/journal/pubdates for revised estimates.
岩浆中的气泡形成
火山爆发是由气泡驱动的,当挥发性物质从岩浆中析出时形成气泡。气泡形成的条件主要取决于岩浆的组成、挥发性浓度、结晶的存在和岩浆的减压速率。这些都是基于挥发性物质从熔体中析出形成气泡的机制。我们批判性地回顾了已知的或推断的岩浆气泡形成机制:均匀成核,晶体表面的非均匀成核和自发相分离(spinodal分解)。我们提出了一种计算气泡成核率的一般方法,即均相成核和非均相成核的贡献之和,这表明在爆发之前,成核可能并不局限于单一的机制。我们确定了三个主要挑战,其中需要进一步的实验,分析和理论工作,以允许在自然喷发条件下形成气泡的一般模型的发展。▪我们回顾了岩浆中气泡形成的机制,并总结了各种机制被理解运作的条件。▪气泡的形成机制可能在岩浆上升过程中随着条件的变化而演变,气泡可能通过多种机制同时和依次形成。▪多相晶体相的均相成核和非均相成核的贡献可以通过一个方程来捕获。▪未来的工作应侧重于限制宏观表面张力,表征微物理,并开发一个通过所有机制,在天然岩浆上升路径上模拟气泡形成的一般框架。《地球与行星科学年鉴》第51卷的最终在线出版日期预计为2023年5月。修订后的估计数请参阅http://www.annualreviews.org/page/journal/pubdates。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Annual Review of Earth and Planetary Sciences
Annual Review of Earth and Planetary Sciences 地学天文-地球科学综合
CiteScore
25.10
自引率
0.00%
发文量
25
期刊介绍: Since its establishment in 1973, the Annual Review of Earth and Planetary Sciences has been dedicated to providing comprehensive coverage of advancements in the field. This esteemed publication examines various aspects of earth and planetary sciences, encompassing climate, environment, geological hazards, planet formation, and the evolution of life. To ensure wider accessibility, the latest volume of the journal has transitioned from a gated model to open access through the Subscribe to Open program by Annual Reviews. Consequently, all articles published in this volume are now available under the Creative Commons Attribution (CC BY) license.
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